Geologic mapping of candidate source craters for martian meteorites

Notes: Data source from [9]. Dust Cover Index (DCI) of the crater shown as a deviated value from 1 where 1 is considered dust-free [13]. Relative preservation of the crater as defined by [5,9], respectively – Preservation is scaled from 1-5 with 5 being the most well-preserved and degradation is scaled from 1-4 with 4 being the most well-preserved. Surface unit as described by [11,12], respectively. GEOLOGIC MAPPING OF CANDIDATE SOURCE CRATERS FOR MARTIAN METEORITES. J. S. Hamilton, C. D. K. Herd, E. L. Walton, and L. L. Tornabene, Department of Earth and Atmospheric Sciences, 1-26 Earth Sciences Building, University of Alberta, Edmonton, Alberta, Canada, T6G 2E3, jhamilto@ualberta.ca, Department of Physical Sciences, MacEwan University, Edmonton, Alberta, Canada, Centre for Planetary Science and Exploration/Department of Earth Sciences, University of Western Ontario, London, Ontario, Canada